Goals for learning in Chapter 4 Lecture 3 Matter and Energy

Similar documents
14-Feb-18 INSIDE STARS. Matter and Energy. Matter and Energy. Matter and Energy. What is matter?

4.2 A Scientific View of Energy Kinetic Energy

Chemistry Physical, Chemical, and Nuclear Changes

The (Almost) Modern Atom Model. SUMMARY from previous lecture Energy comes in different forms. ENERGY IS ALWAYS CONSERVED.

Today HW#4 pushed back to 8:00 am Thursday Exam #1 is on Thursday Feb. 11

15.1 Energy and Its Forms. Energy and Work. How are energy and work related? Energy is the ability to do work. Work is a transfer of energy.

Michael Fowler, UVa Physics, 12/1/07. Momentum has Direction

Energy. on this world and elsewhere. Instructor: Gordon D. Cates Office: Physics 106a, Phone: (434)

Chapter 5 Light and Matter: Reading Messages from the Cosmos. What is light? Properties of Waves. Waves. The Electromagnetic Spectrum

Chapter 3. States of Matter

Matter. Energy- which is a property of matter!! Matter: anything that takes up space and has mass

Convection causes granules. Photosphere isn t actually smooth! Granules Up-Close: like boiling water. Corona or of the Sun. Chromosphere: sphere of

What makes the color pink? Black and white TV summary. Different color phosphors. Color TV. Different color pixels

Energy, Work, and Power

INTRODUCTION TO LESSON CLUSTER 7

Everything in the universe can be classified as either matter or energy. Kinetic Energy Theory: All particles of matter are in constant motion.

Sun s Properties. Overview: The Sun. Composition of the Sun. Sun s Properties. The outer layers. Photosphere: Surface. Nearest.

q = m. C p. T q = heat (Joules) m = mass (g) C p = specific heat (J/g.o C) T = change in temp. ( o C) UNIT 11 - SOLIDS, LIQUIDS, & PHASE CHANGES

But what is energy? And what is matter?

STATES OF MATTER. The Four States of Ma/er. Four States. Solid Liquid Gas Plasma

4 Discuss and evaluate the 5th state of matter. 3 - Differentiate among the four states of matter in terms of energy,

Energy: Forms and Changes

THE PHASES OF MATTER. Solid: holds its shape and does not flow. The molecules in a solid vibrate in place, but on average, don t move very far.

States of Matter 1 of 21 Boardworks Ltd 2016

Nuclear Physics. Final Paper and Presentation

Announcement. Station #2 Stars. The Laws of Physics for Elementary Particles. Lecture 9 Basic Physics

Physics 115 Future Physics Midterm Review Exam will be closed book; no calculators; no computers.

Unit 1: Energy and Motion

Unit 4 - Energy & Heat SOL PS.6,7

Hydrogen Lines. What can we learn from light? Spectral Classification. Visible Hydrogen Spectrum Lines: Series. Actual Spectrum from SDSS

Droplets and atoms. Benjamin Schumacher Department of Physics Kenyon College. Bright Horizons 35 (July, 2018)

ET: Astronomy 230 Section 1 MWF Astronomy Building. Outline. The Early Universe? HW1 due today!

Physics Application Overview

Our sole source of light and heat in the solar system. A very common star: a glowing g ball of gas held together by its own gravity and powered

Energy. Potential Kinetic

Today. Exam 1. The Electric Force Work, Energy and Power. Comments on exam extra credit. What do these pictures have in common?

Holding the Nucleus Together

Name Class Date. Energy Energy

The SI unit for Energy is the joule, usually abbreviated J. One joule is equal to one kilogram meter squared per second squared:

The Story of Energy. Forms and Functions

Chemistry A: States of Matter Packet Name: Hour: Page!1. Chemistry A States of Matter Packet

Particle Model of Matter. AQA Physics topic 3

Energy: Forms and Changes

Ch(3)Matter & Change. John Dalton

Nuclear Weapons (and Energy)

What kinds of energy do you see?

Newton s Laws of Motion

Agenda. Chapter 10, Problem 26. All matter is made of atoms. Atomic Structure 4/8/14. What is the structure of matter? Atomic Terminology

UNIT 2 MECHANICS CHAPTER 6 ENERGY

The Sun. The Chromosphere of the Sun. The Surface of the Sun

Unit 5: Energy (Part 2)

Newton s Law of Gravity. Isaac Newton ( ) Newton s Law of Gravity. Newton s Laws of Motion. Newton s Laws of Motion 2/17/17

Light and Matter: Reading Messages from the Cosmos Pearson Education, Inc.

Energy and the Environment. HNRS 228 Spring 2010 Prof. Geller

How does the Sun shine? What is the Sun s structure? Lifetime of the Sun. Luminosity of the Sun. Radiation Zone. Core 3/30/17

When liquid water crystallizes it has six sides. Create a snowflake with six sides.

Energy: Forms and Changes

Chapter 5 Light and Matter: Reading Messages from the Cosmos

STATES OF MATTER. Chapter 3

F=ma. Exam 1. Today. Announcements: The average on the first exam was 31/40 Exam extra credit is due by 8:00 am Friday February 20th.

Chapter 14: Liquids and Solids

This chapter covers all kinds of problems having to do with work in physics terms. Work

Highlights of chapter 5, section 2

Foundations of Physical Science. Unit 2: Work and Energy

Lecture 5: Forces Readings: Section 4-7, Table 29-1

Lecture 21. Temperature. Thermal Expansion. Heat and Internal Energy. Cutnell+Johnson: , Temperature

2 nd Term Worksheet [ ] Subject Physics Class VIII Name : Sec. :

Chapter 5: Light and Matter: Reading Messages from the Cosmos

SPH3U UNIVERSITY PHYSICS

Chapter 23 Changes of Phase. Conceptual Physics Chapter 23 1

Lesson 2 Changes in State

Kinetic Theory of Matter notes 2012

The lower the energy of a substance, the interaction between its atoms and molecules.

Do Now 10 Minutes Topic Free Fall

Chapter 14 Our Star Pearson Education, Inc.

Matter & Energy. Kinetic Theory of Matter. Kinetic Theory of Matter. Kinetic Theory of Matter. Kinetic Theory of Matter. Temperature.

Nuclear Fission. Conceptual Physics 11 th Edition. Nuclear Fission. Nuclear Fission. Nuclear Fission. This lecture will help you understand:

When liquid water crystallizes it has six sides. Create a snowflake with six sides.

Gravitational potential energy

CHM Solids, Liquids, and Phase Changes (r15) Charles Taylor 1/9

Today is Thursday, May 5 th, 2016

Practice Packet: Energy. Regents Chemistry: Dr. Shanzer. Practice Packet. Chapter 4: Energy.

Light and Matter: Reading Messages from the Cosmos. White light is made up of many different colors. Interactions of Light with Matter

Physical Science midterm study guide. Chapter 1 and 2

! Exam 1 in this classroom in 1 week (Oct 1 st )! 40 Multiple choice questions! Will cover material up to and including today.!

Duncan. Q = m. C p. T. Q = heat (Joules) m = mass (g) C p = specific heat capacity (J/g.o C) T = change in temp. ( o C)


Introduction to Energy Study Guide (also use your notes!!!!)

LECTURE 25 NUCLEAR STRUCTURE AND STABILITY. Instructor: Kazumi Tolich

Phase Changes. Measuring temperature during phase changes

Nuclear Chemistry Lecture Notes: I Radioactive Decay A. Type of decay: See table. B. Predicting Atomic Stability

Chapter 5 Light and Matter: Reading Messages from the Cosmos. 5.1 Light in Everyday Life. How do we experience light?

CHAPTER 1 Matter in our Surroundings CONCEPT DETAILS

Elements of Physics II

The Physics of Renewable Energy. By Harold A. Associate Professor Observatory Director NASA/JPL Solar System Ambassador

Midterm 2 PRS Questions

Do Now Monday, January 23, 201

Chapter Preview. Improving Comprehension

What is it? What are the different types?

Wiley Plus Reminder! Assignment 1

Transcription:

Goals for learning in Chapter 4 Lecture 3 Matter and Energy Reading: Chapter 4 Reminder: 20min Quiz on Thursday from Lecture 1,2,3. What s energy? Scientific view Conservation of energy What s matter? Atoms Phases Understanding energy and matter is crucial to understanding the Universe. Units of Energy Perhaps the most familiar units of energy in daily life is Calories. A typical male adult uses about 2,500 Calories of enegy each day. In science, we use Joules. 1 Calorie = 4,184 Joules Watts are the units of energy (measured in joules) consumed per second. 1 Watt = 1 Joule per second 40-watt light bulbs consume 40 joules per second, or about 1/105 calories per second. Therefore, in order to consume the enegy used by a male each day, you will need to turn on a 40-watt bulb for about 260,000 seconds, or 3 days! Forms of Energy Kinetic Energy : Energy of Motion Thermal Energy : Energy of Heat Potential Energy : Energy of Force Gravitational Electric Magnetic Mass Energy : Energy of Stuff Einstein s formula

Kinetic Energy The faster, the heavier the more energy! Kinetic Energy of a moving object is given by a half of its mass times (velocity of motion) 2 E kinetic = (1/2) m v 2 Maurice Greene: weighs 80kg(=m), runs 100m for 9.79 sec His velocity is calculated as v = 100m/(9.79 sec) = 10.2m/sec Now we know his mass and velocity; thus, his kinetic energy is E kinetic = (1/2)*80*(10.2) 2 = 4160 Joules ~ 1 Calorie If he could run twice as faster, then his kinetic energy would be A: 2, B: 4, C: 8 times larger. Thermal Energy What s causing heat? A: Thermal energy Example: Air The air contains numerous microscopic particles, each having its own mass and velocity and moving randomly -- each has kinetic energy of E kinetic =(1/2)m v 2 The average kinetic energy of particles determines temperature of the air. The higher the temperature, the faster the particles move in the air. Thermal energy is simply the sum of kinetic energy of all particles. Suppose that there are N particles: E thermal = N E kinetic = (1/2)N m v 2 Temperature and Heat Temperature measures the average kinetic energy. So, if 10 particles had the same kinetic energy E 1, then temperature would also be given by E 1. Heat is, on ther other hand, given by thermal energy, or the total kinetic energy of all particles. Therefore, heat is given by 10E 1 as opposed to E 1. Using this fact, the book explains why boiling water could be more dangerous than a cooking oven. Potential Energy When forces act on a substance, it acquires potential energy. Example: gravitational force acting on a ball (mass m) at height h from the ground. E gravity = m g h g is the gravitational acceleration. g = 9.8 m/s 2 on Earth Maurice Greene (80kg=m) falls from the top of 5-m(=h) high building (oops!) E gravity = m g h = 80*9.8*5 = 3920 Joules ~ 1 Calorie If he had fallen from 10-m high building (oooops!), then potential energy would be A: 2, B: 4, C: 6 times larger.

Potential --> Kinetic Energy As Maurice Greene falls, he acquires speed. The potential energy is converted to the kinetic energy!! When he hits the ground, the potential energy is zero (because height, h, is zero). Where did the energy go? All the energy was converted into the kinetic energy: Before he fell from the 5-m building, he had about 1 Calorie of potential energy. By the time he hits the ground, he has converted 1 Calorie of potential energy into 1 Calorie of kinetic energy; thus, he hits the ground at velocity of 10m/s, as if he were running 100m at his best time. The conversion and conservation of energy explain many physical phenomena. (The book -- throwing a ball ) Mass Energy You ve got enormous energy! E mass = m c 2 c = 300,000,000 meter per second (m/s) Compare it to: E kinetic =(1/2)m v 2 for Mr. Greene s best speed, v ~ 10 m/s Since velocity of light is so large, the mass energy is enormous: some 60,000,000 times larger for Mr. Greene. A small mass can be a gigantic source of energy. Ultimate source of energy, or Disaster? Applications of the mass energy includes: Nuclear fission ---> Nuclear power plants Nuclear fusion ---> Atomic bombs It s Einstein s finding. How do you think he felt about his finding after Hiroshima? Stars shine by energy from nuclear fusion. It is E mass = m c 2 that makes stars shine. The Material World Matter in different phases: Solid Liquid Gas Plasma Why are there such phases? Atomic structure Thermal energy

Atomic Structure: Protons(+), Neutrons(0), Electrons(-) At a solid phase, molecules are held tightly together (low thermal energy). As temperature is raised, the thermal motion of molecules within a solid becomes more active, partially breaking bond between molecules --> a liquid state (medium thermal energy). A liquid state becomes a gas state for higher temperature (high thermal energy). A gas state becomes a plasma state for very high temperature. Even atoms are broken up into protons, neutrons and electrons. Phase transition ain t instantaneous Evaporation and Sublimation Atoms and molecules are always trying to free themselves up! Constant escape of molecules from a solid: sublimation Constant escape of molecules from a liquid state: evaporation

20min Quiz on Thursday 11 Multiple-choice Problems you choose the right answer from multiple choices (a) through (d). Problems will be chosen from Does It Make Sense? at the end of each chapter. Make sure that you know not only yes or no, but also why it is yes or no. (There will be two yes and two no in multiple choices!) 3 problems from Chapter 1 4 problems from Chapter 2 4 problems from Chapter 4 2 Short-answer Problems you answer in short sentences. 1 problem from Chapter 2 on eclipses. 1 problem from Chapter 4 on conservation of energy.